Libration points in the restricted three-body problem: Euler angles, existence and stability

Hadia H. Selim; Juan L. G. Guirao; Elbaz I. Abouelmagd

doi:10.3934/dcdss.2019044

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2019, Volume 12, Issue 4&5: 703-710. Doi: 10.3934/dcdss.2019044 open access

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Libration points in the restricted three-body problem: Euler angles, existence and stability

1.
Celestial Mechanics Unit, Astronomy Department, National Research Institute of Astronomy and Geophysics (NRIAG), Helwan 11421, Cairo, Egypt
2.
Departamento de Matemática Aplicada y Estadística, Universidad Politécnica de Cartagena, Hospital de Marina, 30203-Cartagena, Región de Murcia, Spain
3.
Nonlinear Analysis and Applied Mathematics Research Group (NAAM), Mathematics Department, King Abdulaziz University, Jeddah, Saudi Arabia
4.
Celestial Mechanics Unit, Astronomy Department, National Research Institute of Astronomy and Geophysics (NRIAG), Helwan 11421, Cairo, Egypt

* Corresponding author: Elbaz I. Abouelmagd
* Corresponding author: Elbaz I. Abouelmagd

Received: April 30, 2017

Revised: December 31, 2017

Published: March 2019

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Abstract

The objective of the present paper is to study in an analytical way the existence and the stability of the libration points, in the restricted three-body problem, when the primaries are triaxial rigid bodies in the case of the Euler angles of the rotational motion are equal to $ θ_i = π/2, \, ψ_i = 0, \,\varphi_i = π/2 $, $ i = 1, 2 $. We prove that the locations and the stability of the triangular points change according to the effect of the triaxiality of the primaries. Moreover, the solution of long and short periodic orbits for stable motion is presented.

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Mathematics Subject Classification: Primary: 2010; Secondary: 37N05, 70F15.

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